LeMMINGs VII: 5 GHz, 50 mas e-MERLIN observations of a statistically complete sample of nearby AGN
D. R. A. Williams-Baldwin (1), R. D. Baldi (2), R. J. Beswick (1), I. M. McHardy (3), E. Carver (3), J. Clifford (3), B. T. Dullo (4), N. Kill (3), B. Krishnamoorthi (3), I. M. Mutie (5, 1), O. Woodcock (1), M. K. Argo (6), P. Boorman (7), E. Brinks (8), D. M. Fenech (9)

TL;DR
This study uses high-resolution 5 GHz e-MERLIN radio imaging to analyze nuclear activity in a complete sample of nearby galaxies, revealing that a significant fraction host compact radio cores indicative of active galactic nuclei.
Contribution
First high-resolution 5 GHz e-MERLIN survey of a complete local galaxy sample, providing new insights into low-luminosity AGN prevalence and characteristics.
Findings
24% of galaxies show nuclear radio emission
Most detections are compact (<10 pc)
Up to 30% of local galaxies host radio-active nuclei
Abstract
We present 5 GHz e-MERLIN radio images at 50 mas resolution of the nuclear regions of the Legacy e-MERLIN Multi-band Imaging of Nearby Galaxies survey (LeMMINGs), the deepest statistically complete radio-band survey of the local Universe (<120 Mpc), consisting of 280 galaxies spanning all morphological and nuclear types. We detect nuclear radio emission above a median 5 sigma threshold of 0.33 mJy beam^-1 in 68 of 280 sources (24 percent), with core luminosities in the range 10^35 to 10^41.9 erg s^-1. The radio emission is attributed to active galactic nuclei, circumnuclear star formation, or, in the case of NGC 3690, a tidal disruption event. The brightest radio nuclei, with brightness temperatures >=10^6 K, reside in optically active galaxies such as LINERs and Seyferts. The detection rate for inactive systems (H II and absorption-line galaxies), which may host low-luminosity active…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Radio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena
